Oxygen's ups and downs in the early atmosphere and ocean

Oct 23, 2012

This is a carbonate rock in Zimbabwe used to trace sulfate levels in the Earth's early oceans. Credit: Lyons Lab, UC Riverside

Most researchers imagine the initial oxygenation of the ocean and atmosphere to have been something like a staircase, but with steps only going up. The first step, so the story goes, occurred around 2.4 billion years ago, and this, the so-called Great Oxidation Event, has obvious implications for the origins and evolution of the first forms of eukaryotic life. The second big step in this assumed irreversible rise occurred almost two billion years later, coinciding with the first appearances and earliest diversification of animals.

Now a team led by geochemists at the University of California, Riverside challenges the simple notion of an up-only trend for early oxygen and provides the first compelling direct evidence for a major drop in oxygen after the first rise.

"Our group is among a subset of scientists who imagine that oxygen, once it began to accumulate in the ocean-atmosphere system, may have ultimately risen to very high levels about 2.3-2.2 billion years ago, perhaps even to concentrations close to what we see today," said Timothy Lyons, a professor of biogeochemistry and the principal investigator of the project. "But unlike the posited irreversible rise favored by many, our new data point convincingly to an equally impressive, and still not well understood, fall in oxygen about 200 million years later."

According to Lyons, this drop in oxygen may have ushered in more than a billion years that were marked by a return to low-oxygen concentrations at Earth's surface, including the likelihood of an oxygen-free deep ocean.

"It is this condition that may have set the environmental stage and ultimately the clock for the advance of eukaryotic organisms and eventually animals," he said.

"The time window between 2.3 and 2.1 billion years ago is famous for the largest and longest-lived positive carbon isotope excursion in Earth history," said Noah Planavsky, a recent Ph.D. graduate from UC Riverside, current postdoctoral fellow at Caltech, and first author of the research paper.

He explained that carbon isotopes are fractionated during photosynthesis. When organic matter is buried, oxygen is released and rises in the biosphere. The burial of organic matter is tracked by the positive or heavy isotopic composition of carbon in the ocean.

"Some workers have attributed the carbon isotope excursion to something other than organic burial and associated release of oxygen," Planavsky said. "We studied the sulfur isotope composition of the same rocks used for the carbon isotope analyses—from Canada, South Africa, the U.S., and Zimbabwe—and demonstrated convincingly that the organic burial model is the best answer."

The researchers' sulfur data point to high sulfate concentrations in the ocean, which, like today, is a classic fingerprint of high oxygen levels in the ocean and atmosphere. Sulfate, the second most abundant negatively charged ion in the ocean today, remains high when the mineral pyrite oxidizes easily on the continents and is buried in relatively small amounts in the oxygen-rich ocean.

"What is equally impressive is that the rise in oxygen was followed by a dramatic fall in sulfate and therefore oxygen," Lyons said. "Why the rise and fall occurred and how that impacted the billion years or more of ocean chemistry that followed and the life within that ocean are hot topics of research."

The research team is thrilled to have found strong chemical evidence for oxygen variability on the early Earth.

"The idea that oxygen levels at Earth's surface went up and down must be vital in any effort to understand the links between environmental and biological evolution on broad, geologic time scales," Planavsky said.

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User comments : 4

I'd like to see some analysis of how atmospheric pressure/density has varied over time. How else to explain flying creatures like: dragonfiles w/2' wingspan, pterodactyls w/20' wingspan. Why don't we see anything like that today? Was the atmosphere more dense then? How would you go about determining that?

Roland, you're probably correct that atmospheric pressure at sea level has varied. Gases are (very slowly) lost to space and replenished by volcanic processes, the latter being characterized by intermittant surges of activity.

But fluctuations in atmospheric density *ought* to have been fairly small over the past 2.2 billion years, and of little significance to aerodynamics.

Insect size is constrained, not by aerodynamics, but two completely different factors: atmospheric O2 content (higher concentrations of O2 permit larger insects) and predation. Fairly recently, a study was reported here which correlated the rise of birds with insect shrinkage. Big bugs were too easy to catch and suffered a natural selection penalty, once birds arrived on the scene.

Predation is probably the reason no large flying animals have arisen to replace large flying reptiles after their extinction. Mammals are too quick and too clever; birds needed to go smaller to succeed, and they have.

Birds are also more robust flying machines than animals relying on thin membranes for wings. bird feathers overlap, and the gap caused by loss of one feather is immediately repaired by the next feather, since feathers have miniature "hooks".A predatory bird can thus attack targets approaching its own size without major risk of wing damage.

@Urgelt: "But fluctuations in atmospheric density *ought* to have been fairly small over the past 2.2 billion years"

Why would that be? Venus is smaller than Earth w/less G, and is losing its atmosphere rapidly. It's the only planet with a tail like a comet. Yet its surface pressure is ~90 bar. So LARGE pressure variations w/time are possible.

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